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FEATURED STORY

FEATURED STORY

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Laboratory News

Congratulations to Charles Bennett, Gary Hinshaw, Norman Jarosik, Lyman Page Jr., David Spergel and the WMAP Science Team for winning the 2018 Breakthrough Prize in Fundamental Physics

12.03.2017
Congratulations to Charles Bennett, Gary Hinshaw, Norman Jarosik, Lyman Page Jr., David Spergel and the WMAP Science Team for winning the 2018 Breakthrough Prize in Fundamental Physics on Dec. 3! The citation reads: “For detailed maps of the early universe that greatly improved our knowledge of the evolution of the cosmos and the fluctuations that seeded the formation of galaxies.” The Breakthrough Prize in Fundamental Physics was founded in 2012 by Yuri Milner to recognize those individuals who have made profound contributions to human knowledge. The team also includes:

Chris Barnes, Olivier Doré, Joanna Dunkley, Ben Gold, Michael Greason, Mark Halpern, Robert Hill, Al Kogut, Eiichiro Komatsu, David Larson, Michele Limon, Stephan Meyer, Michael Nolta, Nils Odegard, Hiranya Peiris, Kendrick Smith, Greg Tucker, Licia Verde, Janet Weiland, Ed Wollack, and Ned Wright

Congratulations to the many ASD members who were involved in the exciting gravitational wave and electromagnetic counterpart discovery of merging neutron stars, and the subsequent media activity around the discovery!

10.23.2017
Scientists:

Scott Barthelmy - Gamma-ray Coordinates Network system
Eric Burns - Fermi gamma ray burst study
Jordan Camp – GSFC LIGO Scientific Collaboration (LSC) PI
Brad Cenko - Swift PI
Tito Dal Canton - Gravitational wave localization maps; Virgo, joint LIGO/Virgo-Fermi-GBM study
Amy Lien - Swift follow up study
Julie McEnery - Fermi Project Scientist
Frank Marshall - Swift follow up study
Judy Racusin - Fermi gamma ray burst study, Swift follow-up study
Leo Singer - Gravitational wave localization maps, GROWTH follow-up study, joint LIGO/Virgo-Fermi-GBM study
Eleonora Troja - Chandra & HST follow-up, Swift follow-up study

Communications Team:

Elizabeth Ferrara - Fermi social media
Barb Mattson - Traditional & social media coordination
Sara Mitchell - Social media coordination & content creation
Brian Monroe - Animator
Frank Reddy - Cross-organizational coordination & writer for nasa.gov press release
Claire Saravia - Live shots
Amber Straughn - ASD Associate Director
Dewayne Washington - HQ/GSFC coordination
Scott Wiessinger - Video & multimedia

Congratulations to the Astrophysics Science Division scientists who are PIs and Co-Is on the recently announced Astrophysics Missions of Opportunity and Medium-Class Explorer missions!

08.09.2017
  • ISS-TAO (Transient Astrophysics Observer on the ISS), a Mission of Opportunity proposal submitted to the 2016 Explorer opportunity, was selected for a Phase A study. ISS-TAO team members include PI Jordan Camp (663), Scott Barthelmy (661), Rob Petre (662), Judy Racusin (661), Brad Cenko (661), Frank Marshall (661), Jeremy Schnittman (663), Andy Ptak (662), and Amy Lien (661), Leo Singer (661), and Tod Strohmeyer (662). ISS-TAO is a wide-field X-ray transient detector aboard the International Space Station that would observe numerous events per year of X-ray transients related to compact objects. The mission’s primary goal is the detection of X-ray counterparts to gravitational waves produced by neutron stars merging with black holes and other neutron stars. Other targets would be supernova shocks, neutron star bursts, and high redshift gamma-ray bursts.
  • Rob Petre (662), Andy Ptak (662), Alan Smale (660), and Lynne Valencic (662) are co-Is on Arcus (PI Randall Smith, SAO), selected as a concept study for a Medium-Class Explorer mission. Arcus would study stars, galaxies and clusters of galaxies using high-resolution X-ray spectroscopy to characterize the interactions between these objects and the diffuse million-degrees gas that surrounds and permeates them.
  • Alan Smale (660) and Terri Brandt (661) are collaborators on COSI-X (PI Steve Boggs/UCB), selected as a concept study for an Explorer Mission of Opportunity. COSI-X is a balloon-borne, wide-field-of-view telescope designed to survey the gamma-ray sky at 0.2-5 MeV, performing high-resolution spectroscopy, wide-field imaging, and polarization measurements. COSI-X would map gamma-rays from antimatter around the Milky Way's center, as well as from newly-formed radioactive elements in the debris of stellar explosions.
The NASA press release announcing the selections is here: https://www.nasa.gov/press-release/nasa-selects-proposals-to-study-galaxies-stars-planets
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Overview

The X-ray Astrophysics Laboratory conducts investigations of a broad range of astronomical systems through detection and analysis of their X-ray emission and other radiation they emit. Objects studied range from nearby solar system objects to cosmological structures. Researchers at the Laboratory investigate the physics of extreme environments, such as those near the event horizons of black holes, and the evolution of stars, galaxies, and large-scale structures.

The Laboratory is the preeminent developer of state-of-the-art X-ray astronomical detectors and optical systems for performing precise spectroscopy, polarimetry, timing, and imaging. These instruments have been employed in numerous suborbital applications (sounding rockets and balloons) and orbiting observatories.

Read a history of X-ray astronomy at Goddard.

Contact Us

Dr. Robert Petre
301.286.3844
Chief [662]
Dr. Joanne E. Hill-Kittle
301.286.0572
Associate Lab Chief [662]
Renita B Springs
301.286.9662
Project Support Specialist [662]
                                                                                                                                                                                        
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